Cooling of Accretion-Heated Neutron Stars
作者： Nathalie Degenaar , Rudy Wijnands , Dany Page
DOI: 10.1007/S12036-017-9466-5
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摘要: We present a brief, observational review about the study of cooling behaviour accretion-heated neutron stars and inferences neutron-star crust core that have been obtained from these studies. Accretion matter during outbursts can heat out thermal equilibrium with after accretion episodes are over, will cool down until crust-core is restored. discuss observed properties sources what has learned physics crusts. also briefly those systems long their were i.e, times when expected to be in equilibrium. The surface temperature then direct probe for temperature. By comparing temperatures based on estimates history targets ones, cores investigated. Finally, we similar studies performed strongly magnetized which magnetic field might play an important role heating stars.
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